Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baicz..33..215b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin, vol. 33, no. 4, 1982, p. 215-219.
Astronomy and Astrophysics
Astronomy
2
Geomagnetism, Magnetic Field Configurations, Solar Activity Effects, Solar Flares, Solar Protons, Sunspots, Magnetic Disturbances, Solar Atmosphere, Solar Corona, Solar Terrestrial Interactions, Solar Wind
Scientific paper
Characteristics of the solar wind emanating from the region of the solar atmosphere in which the formation of the June-July 1974 proton-flare region took place are investigated. It is shown that the daily geomagnetic character figures C 9 reach their maximum when the rapid disintegration and disappearance of the large-scale characteristic magnetic field patterns occur and when there is a sudden cessation of sunspot, flare, and coronal activity. This solar wind enhancement is taken as one of the last observable manifestations of the entire complex process.
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